The DESI Bright Galaxy Survey: Final Target Selection, Design, and Validation
Over the next 5 yr, the Dark Energy Spectroscopic Instrument (DESI) will use 10 spectrographs with 5000 fibers on the 4 m Mayall Telescope at Kitt Peak National Observatory to conduct the first Stage IV dark energy galaxy survey. At z < 0.6, the DESI Bright Galaxy Survey (BGS) will produce the mo...
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Médium: | Článek |
Jazyk: | English |
Vydáno: |
IOP Publishing
2023-01-01
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Edice: | The Astronomical Journal |
Témata: | |
On-line přístup: | https://doi.org/10.3847/1538-3881/accff8 |